File:ML-star.png

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Original file (1,621 × 1,508 pixels, file size: 129 KB, MIME type: image/png)

Summary

Description
English: Illustration of the Mittag-Leffler star (the region bounded by the blue contour). The original disk U is centered at a.
Русский: Изображение звезды Миттаг-Леффлера (область, ограниченная синим контуром). Изначальный диск U {\displaystyle U} имеет центр в точке a {\displaystyle a}.
Date
Source Own work
Author Oleg Alexandrov
PNG development
InfoField
 This diagram was created with MATLAB.

Licensing

Public domain This work has been released into the public domain by its author, Oleg Alexandrov. This applies worldwide.
In some countries this may not be legally possible; if so:
Oleg Alexandrov grants anyone the right to use this work for any purpose, without any conditions, unless such conditions are required by law.

Source code (MATLAB)

 

function main()

%   Illustration of the Mittag-Leffler star
   
   lw=3.0;
   lightblue = [0.8 0.8 1];
   red=[0.867 0.06 0.14];
   blue = [0, 129, 205]/256;
   green = [0, 146,  70]/256;
   white=0.99*[1, 1, 1];
   
   % will draw a spline-interpolated curve through these points
   XX=[0.0543 -0.4058 -0.8211 -0.5463 -0.1310  0.1821  0.5847  0.2907];
   YY=[0.7796  0.3578  0.1661 -0.1597 -0.5495 -0.2748 -0.1278  0.3323];

   figure(2); clf; hold on; axis equal; axis off;
   N=100; % how fine to make the interpolation
   [X, Y] = get_spline(N, XX, YY);
   plot(X, Y, 'LineWidth', lw, 'color', blue);
   
%  the number of circles to plot and their radii
   P = 6; R=1:P; R=1.09-1./R.^1.3; R=[0  0.4 R(2:length(R))];
   M=length(R);

%  plot rays
   O=[0, 0]; 
   Angles=[1.0 2.34 6.1];
   for l=1:length(Angles)
	  m = floor(Angles(l)*N)+1;
	  E = [X(m), Y(m)];
   
	  plot([O(1), E(1)], [O(2), E(2)], 'linewidth', lw, 'color', green);
   end;
   
   % plot central circle and its center
   radius=0.2; 
   plot_circle(O(1), O(2), radius, lw, red);
   tinyrad = 0.013;
   ball(O(1), O(2), tinyrad, green);

   % plot circles along the rays
   for l=1:length(Angles)
	  m = floor(Angles(l)*N)+1;
	  E = [X(m), Y(m)];
   
	  e=norm(E);
	  for i=2:(M-1)
		 t=R(i);
		 radius=0.85*(R(i+1)-R(i))*e;
		 C=t*E;
		 plot_circle(C(1), C(2), radius, lw, red);
	  end
   end


%  text
   fontsize = 26;
   tiny=0.0022*fontsize;
   text(O(1)-tiny, O(2)-tiny, '\it{a}', 'fontsize', fontsize);

%   plot a box around the figure to avoid bugs with saving to eps
   offset=0.04;
   plot(min(X)-offset, min(Y)-offset, '*', 'color', white)
   plot(max(X)+offset, max(Y)+offset, '*', 'color', white)

   saveas(gcf, 'ML-star.eps', 'psc2')
%  to later convert from eps to png use
%  convert -antialias -density 250 ML-star.eps ML-star.png
   
function [xx, yy] = get_spline(N, x, y)
   
   n=length(x); 
   P=5; Q=n+2*P+1; % P will denote the amount of overlap
   
% Make the 'periodic' sequence xp=[x(1) x(2) x(3) ... x(n) x(1) x(2) x(3) ... ]
% of length Q. Same for yp.
   for i=1:Q
	  j=rem(i, n)+1; % rem() is the remainder of division of i by n
	  xp(i)=x(j);
	  yp(i)=y(j);
   end
   
% do the spline interpolation
   t=1:length(xp);
   tt=1:(1/N):length(xp);
   xx=spline(t, xp, tt);
   yy=spline(t, yp, tt);
   
% discard the redundant pieces
   start=N*(P-1)+1;
   stop=N*(n+P-1)+1;
   xx=xx(start:stop); 
   yy=yy(start:stop);

function plot_circle(x, y, r, lw, color)

   Theta=0:0.1:2.1*pi;
   X=r*cos(Theta)+x;
   Y=r*sin(Theta)+y;
   plot(X, Y, 'linewidth', lw, 'color', color);

function ball(x, y, r, color)
   Theta=0:0.1:2.1*pi;
   X=r*cos(Theta)+x;
   Y=r*sin(Theta)+y;
   H=fill(X, Y, color);
   set(H, 'EdgeColor', 'none');
This math image could be re-created using vector graphics as an SVG file. This has several advantages; see Commons:Media for cleanup for more information. If an SVG form of this image is available, please upload it and afterwards replace this template with {{vector version available|new image name}}.
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Date/TimeThumbnailDimensionsUserComment
current22:04, 16 April 2007Thumbnail for version as of 22:04, 16 April 20071,621 × 1,508 (129 KB)wikimediacommons>Oleg Alexandrov

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